6533b871fe1ef96bd12d2571
RESEARCH PRODUCT
High-order methods for the simulation of hydromagnetic instabilities in core-collapse supernovae
Ewald MüllerTomasz RembiaszPablo Cerdá-duránM. Angel AloyM. Obergaulingersubject
PhysicsAstronomy and Astrophysics010103 numerical & computational mathematics01 natural sciencesInstabilityRiemann solverNumerical resistivity010305 fluids & plasmasComputational physicsRoe solverSupernovasymbols.namesakeRiemann problemSpace and Planetary Science0103 physical sciencesTearingsymbols0101 mathematicsMagnetohydrodynamicsdescription
AbstractWe present an assessment of the accuracy of a recently developed MHD code used to study hydromagnetic flows in supernovae and related events. The code, based on the constrained transport formulation, incorporates unprecedented ultra-high-order methods (up to 9th order) for the reconstruction and the most accurate approximate Riemann solvers. We estimate the numerical resistivity of these schemes in tearing instability simulations.
| year | journal | country | edition | language |
|---|---|---|---|---|
| 2011-06-08 | Proceedings of the International Astronomical Union |